Temperature
5595 K
5410.7 to 5803
Unclassified star • 1090.5 pc
Records
22
literature rows
Planets
2
system count
References
16
distinct source labels
Approximate color
from effective temperature
Canonical Summary
Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.
Stellar source: Morton et al. 2016 • System source: TICv8
Temperature
5595 K
5410.7 to 5803
Mass
0.93 Msun
0.87 to 0.98
Radius
0.90 Rsun
0.80 to 1.42
Age
4.17 Gyr
0.50 to 10.96
Distance
1090.5 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 0.90 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-373
0.90 R☉
System Layout
2 planets linked to this host
Transit
Discovery
2014
Period
5.54 days
Radius
1.36 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2014
Period
16.73 days
Radius
1.24 R⊕
Mass
—
Eq. Temp
—
Kepler-373 is a star located 3560 light-years away. It hosts two planets, both discovered by transit in 2014. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness; repeated dips help establish orbital periods. The star's reported mass estimate is smaller than the Sun's, and its reported temperature of 5600 K is cooler than the Sun's. It is 0.93 solar masses, 0.9 solar radii, and 4.17 billion years old.
Kepler-373 b and Kepler-373 c are both Earth-like planets, a size class that stays within 1.5 times Earth's radius. Kepler-373 b has an orbital period of 5.54 days and a radius of 1.36 Earth radii. Kepler-373 c orbits every 16.7 days at 1.24 Earth radii. Among the listed planets, Kepler-373 b has the shortest year by reported estimates, while Kepler-373 c has the longest. Kepler-373 b also has the largest radius by reported estimates, and Kepler-373 c the smallest.
Provenance
Evidence Summary
Rows
22
Stellar refs
15
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5783 | 0.90 | 0.84 | — | — | — | 1090.5 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5803 | 0.98 | 0.87 | 0.50 | — | — | 1090.5 | Q1-Q8 KOI Table | TICv8 |
| 5803 | 0.98 | 0.87 | 0.50 | — | — | 1090.5 | Q1-Q8 KOI Table | TICv8 |
| 5783 | 0.90 | 0.84 | — | — | — | 1090.5 | Q1-Q12 KOI Table | TICv8 |
| 5553 | 0.98 | 1.38 | — | 0.21 | — | 1090.5 | TICv8 | TICv8 |
| — | — | — | — | — | — | 1090.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5588 | 0.95 | 1.10 | — | — | — | 1090.5 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5539 | 0.87 | 0.80 | — | — | — | 1090.5 | Batalha et al. 2013 | TICv8 |
| 5539 | — | 0.80 | — | — | — | 1090.5 | Q1-Q6 KOI Table | TICv8 |
| — | — | — | — | — | — | 1090.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5539 | — | 0.87 | — | — | — | 1090.5 | Latham et al. 2005 | TICv8 |
| 5783 | 0.90 | 0.84 | — | — | — | 1090.5 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5539 | — | 0.80 | — | — | — | 1090.5 | Q1-Q6 KOI Table | TICv8 |
| 5410.7 | — | 1.42 | — | 0.19 | — | 1090.5 | Gaia DR2 | TICv8 |
| 5783 | 0.90 | 0.84 | — | — | — | 1090.5 | Q1-Q16 KOI Table | TICv8 |
| 5783 | 0.90 | 0.84 | — | — | — | 1090.5 | Q1-Q12 KOI Table | TICv8 |
| 5783 | 0.90 | 0.84 | — | — | — | 1090.5 | Q1-Q16 KOI Table | TICv8 |
| 5595 | 0.93 | 0.90 | 4.17 | — | — | 1090.5 | Morton et al. 2016 | TICv8 |
| 5602 | 0.98 | 1.33 | 10.96 | — | — | 1090.5 | Fulton & Petigura 2018 | TICv8 |
| 5602 | — | 1.36 | — | — | — | 1090.5 | Berger et al. 2018 | TICv8 |
| 5588 | 0.95 | 1.10 | — | — | — | 1090.5 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5787 | — | 0.84 | — | — | — | 1090.5 | Rowe et al. 2014 | TICv8 |